Searching for planets around eclipsing binary stars using timing method: NSVS 14256825

NASIROĞLU İ., GOZDZIEWSKI K., Slowikowska A., KRZESZOWSKİ K., ZEJMO M., Zola S., ...Daha Fazla

330th Symposium of the International-Astronomical-Union (IAU), Nice, Fransa, 24 - 28 Nisan 2017, cilt.12, ss.405-406 identifier

  • Yayın Türü: Bildiri / Tam Metin Bildiri
  • Cilt numarası: 12
  • Doi Numarası: 10.1017/s1743921317005658
  • Basıldığı Şehir: Nice
  • Basıldığı Ülke: Fransa
  • Sayfa Sayıları: ss.405-406
  • Atatürk Üniversitesi Adresli: Evet

Özet

We present four new mid eclipse times and an updated O-C diagram of the short period eclipsing binary NSVS14256825. The new data follow the (O-C) trend and its model proposed in Nasiroglu et al. (2017). The (O-C) diagram shows quasi-periodic variations that can be explained with the presence of a brown-dwarf in a quasi-circular circumbinary orbit.